A New 24 μm Phase Curve for υ Andromedae b
We report the detection of 24 μm variations from the planet-hosting υ Andromedae system consistent with the orbital periodicity of the system's innermost planet, υ And b. We find a peak-to-valley phase curve amplitude of 0.00130 times the mean system flux. Using a simple model with two hemisphe...
Main Authors: | , , , , , , |
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Other Authors: | |
Format: | Article |
Language: | English |
Published: |
IOP Publishing,
2012-10-19T16:02:03Z.
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Subjects: | |
Online Access: | Get fulltext |